The general solution of the classical equation of motion dμ/dt = g(μ×H)⁠, when H consists of a constant field plus a perpendicular rotating component can easily be obtained after transforming the problem to a properly chosen rotating coordinate system. The value of this method for teaching purposes is discussed.

Topics
Magnetic fields, Properties of nuclei, Teaching
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© 1953 American Association of Physics Teachers.
1953
American Association of Physics Teachers
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